Table 1
Model selection results for object 179.
| Model | L 2−10keV | Γ | N H | KL | NH | log Z | p(M | D) | BIC | AIC |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
|
|
||||||||
| torus+pexmon+scattering |
|
|
|
1.43 | 0.0 | 40.0% | –109.40 | –122.59 |
| sphere+pexmon+scattering |
|
|
|
1.46 | –0.1 | 30.2% | –109.40 | –122.59 |
| wabs+pexmon+scattering |
|
|
|
1.44 | –0.1 | 29.0% | –109.43 | –122.62 |
| torus+scattering |
|
|
|
1.42 | –2.0 | 0.4% | –105.18 | –113.97 |
| sphere+scattering |
|
|
|
1.45 | –2.1 | 0.3% | –105.87 | –114.67 |
| wabs+scattering |
|
|
|
1.44 | –2.7 | 0.1% | –103.08 | –111.88 |
| sphere |
|
|
|
1.52 | –4.7 | 0.0% | –98.07 | –102.47 |
| torus |
|
|
|
1.54 | –4.7 | 0.0% | –97.63 | –102.02 |
| wabs |
|
|
|
1.58 | –5.5 | 0.0% | –95.13 | –99.53 |
| powerlaw |
|
|
–27.9 | 0.0% | 0.00 | 0.00 | ||
Notes. Derived luminosity (logarithmic, in erg/s) (2), photon index (3), and column density (4, logarithmic, in cm-2) are shown with 1σ-equivalent quantile errors (see Fig. 6 for the posterior distributions). The fifth column shows the information gain in column density in ban (see text). The last four columns show the model comparison results based on log-evidence, posterior assuming all models have same prior probability, BIC and AIC.
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